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Fe isotopes and the contrasting petrogenesis of A-, I- and S-type granite

dc.contributor.authorFoden, J
dc.contributor.authorSossi, Paolo
dc.contributor.authorWawryk, Christine
dc.date.accessioned2015-12-13T22:33:10Z
dc.date.issued2015
dc.date.updated2015-12-11T09:14:17Z
dc.description.abstractWe present new Fe isotope data of 42 S-, I- and A-type (ferroan) granites from the Cambrian Delamerian orogen in South Australia, the Palaeozoic Lachlan Fold Belt and Western USA. Interpretation of these data, together with modelling suggests that magmatic processes do result in quite complex Fe-isotopic differentiation trends and can lead to granites with isotopically heavy iron with δ57Fe>0.35‰. By comparison Mid-Ocean Ridge Basalts (MORBs) have δ57Fe=0.15‰ (Teng et al., 2013). These variations are similar to those previously reported (Poitrasson and Freydier, 2005; Heimann et al., 2008; Telus et al., 2012), but, contrary to some interpretations (Beard and Johnson, 2006; Heimann et al., 2008), heavy values are not necessarily the product of late-stage hydrothermal fluid loss, though this process is undoubtedly also an important factor in some circumstances. A-type (ferroan) granites reach very heavy δ57Fe values (0.4-0.5‰) whereas I-types are systematically lighter (δ57Fe=0.2‰). S-type granites show a range of intermediate values, but also tend to be isotopically heavy (δ57Fe≈0.2-0.4‰). Our results show that the iron isotopic values and trends are signatures that reflect granite generation processes. A modelling using the Rhyolite-MELTS software suggests that contrasting trajectories and end-points in Fe isotope evolution towards granite depend on: oxidation state of the evolving magma and, whether or not the system is oxygen-buffered. Iron isotopic evolution supports an origin of ferroan A-type granite from protracted, closed magma chamber fractionation of moderately reduced mafic magmas. In these systems magnetite saturation is delayed and the ferric iron budget is finite. I-type systems originate with the supply of relatively oxidised, hydrous, subduction-related magmas from the mantle wedge to the upper plate crust. These then experience oxygen-buffered open-system AFC processes in lower crustal hot-zones. S-type magmas are crustal melts that crystallise under reduced conditions initially imposed at source by sulphidic or graphitic sedimentary protoliths. The composition of the resulting melts reflects the domination of partial melting where conditions are hence buffered (open system) followed by subsequent late-stage, closed system fractionation of these extracted, reduced magmas.
dc.identifier.issn0024-4937
dc.identifier.urihttp://hdl.handle.net/1885/75896
dc.publisherElsevier
dc.sourceLithos
dc.titleFe isotopes and the contrasting petrogenesis of A-, I- and S-type granite
dc.typeJournal article
local.bibliographicCitation.lastpage44
local.bibliographicCitation.startpage32
local.contributor.affiliationFoden, J., University of Adelaide
local.contributor.affiliationSossi, Paolo, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWawryk, Christine, University of Adelaide
local.contributor.authoruidSossi, Paolo, u4968018
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor040300 - GEOLOGY
local.identifier.ariespublicationU3488905xPUB4844
local.identifier.citationvolume212-215
local.identifier.doi10.1016/j.lithos.2014.10.015
local.identifier.scopusID2-s2.0-84911366561
local.type.statusPublished Version

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